The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. XI. Lupus Observed With IRAC and MIPS
arXiv:0803.1504 · doi:10.1086/588042
Abstract
We present c2d Spitzer/IRAC observations of the Lupus I, III and IV dark clouds and discuss them in combination with optical and near-infrared and c2d MIPS data. With the Spitzer data, the new sample contains 159 stars, 4 times larger than the previous one. It is dominated by low- and very-low mass stars and it is complete down to M 0.1M. We find 30-40 % binaries with separations between 100 to 2000 AU with no apparent effect in the disk properties of the members. A large majority of the objects are Class II or Class III objects, with only 20 (12%) of Class I or Flat spectrum sources. The disk sample is complete down to ``debris''-like systems in stars as small as M 0.2 M and includes sub-stellar objects with larger IR excesses. The disk fraction in Lupus is 70 -- 80%, consistent with an age of 1 -- 2 Myr. However, the young population contains 20% optically thick accretion disks and 40% relatively less flared disks. A growing variety of inner disk structures is found for larger inner disk clearings for equal disk masses. Lupus III is the most centrally populated and rich, followed by Lupus I with a filamentary structure and by Lupus IV, where a very high density core with little star-formation activity has been found. We estimate star formation rates in Lupus of 2 -- 10 M Myr and star formation efficiencies of a few percent, apparently correlated with the associated cloud masses.
Accepted for publication in the ApJS. Contains 101 pages, 23 figures, and 13 tables. A version with full resolution figures can be found at http://peggysue.as.utexas.edu/SIRTF/PAPERS/pap102.pub.pdf
References in corpus (11)
- Dust dynamics during protoplanetary disc clearing
- Binarity as a key factor in protoplanetary disk evolution: Spitzer disk census of the eta Chamaeleontis cluster
- Young, Low-Mass Brown Dwarfs with Mid-Infrared Excesses
- The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds.X. The Chamaeleon II Pre-Main Sequence Population as Observed With IRAC and MIPS
- Empirical isochrones and relative ages for young stars, and the radiative-convective gap
- Medium-separation binaries do not affect the first steps of planet formation
- SPITZER: Accretion in Low Mass Stars and Brown Dwarfs in the Lambda Orionis Cluster
- New Low-Mass Stars and Brown Dwarfs with Disks in Lupus
- Giant Planet Migration in Viscous Power-Law Discs
- The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. IV. Lupus Observed with MIPS
- WWW Database of Models of Accretion Disks Irradiated by The Central Star
Cited by in corpus (42)
- X-Shooter spectroscopy of young stellar objects in Lupus: Accretion properties of class II and transitional objects
- Identifying the Low Luminosity Population of Embedded Protostars in the c2d Observations of Clouds and Cores
- Physical properties of dusty protoplanetary disks in Lupus: evidence for viscous evolution?
- Identification of Young Stellar Object candidates in the DR2 x AllWISE catalogue with machine learning methods
- Bridging the gap between protoplanetary and debris disks: separate evolution of millimeter and micrometer-sized dust
- Multi-wavelength continuum sizes of protoplanetary discs: scaling relations and implications for grain growth and radial drift
- The Nature of Transition Circumstellar Disks II. Southern Molecular Clouds
- MINDS. Abundant water and varying C/O across the disk of Sz 98 as seen by JWST/MIRI
- Measuring the ratio of the gas and dust emission radii of protoplanetary disks in the Lupus star-forming region
- Lupus DANCe. Census of stars and 6D structure with Gaia-DR2 data
- The first ALMA survey of protoplanetary discs at 3 mm: demographics of grain growth in the Lupus region
- Demographics of disks around young very low-mass stars and brown dwarfs in Lupus
- POISSON project - III - Investigating the evolution of the mass accretion rate
- Transition disks: the observational revolution from SEDs to imaging
- A Census of the Circumstellar Disk Populations in the Sco-Cen Complex
- Substellar Objects in Nearby Young Clusters (SONYC) VIII: Substellar population in Lupus 3
- Identification of new transitional disk candidates in Lupus with Herschel
- The effect of stellar multiplicity on protoplanetary discs. A NIR survey of the Lupus star forming region
- ALMA Survey of Lupus Class III Stars: Early Planetesimal Belt Formation and Rapid Disk Dispersal
- Herschel evidence for disk flattening or gas depletion in transitional disks
- Gas inside the 97 au cavity around the transition disk Sz\,91
- A Gaia Survey for Young Stars Associated with the Lupus Clouds
- What happened before? -- The disks around the precursors of young Herbig Ae/Be stars
- Constraining the radial drift of millimeter-sized grains in the protoplanetary disks in Lupus
- ESO-H~574 and Par-Lup3-4 Jets: Exploring the spectral, kinematical and physical properties
- ALMA observations of the Th 28 protostellar disk - A new example of counter-rotation between disk and optical jet
- The Supershell-Molecular Cloud Connection: Large-Scale Stellar Feedback and the Formation of the Molecular ISM
- The ASAS-SN Catalog of Variable Stars VIII: "Dipper" Stars in the Lupus Star-Forming Region
- Dispersal timescale of protoplanetary disks in the low-metallicity young cluster Dolidze 25
- X-Shooter spectroscopy of young stellar objects - VI - HI line decrements
- Outflows, envelopes, and disks as evolutionary indicators in Lupus YSOs
- The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO): III. Dust and Gas Disk Properties in the Lupus Star-forming Region
- Search for Alignment of Disk Orientations in Nearby Star-Forming Regions: Lupus, Taurus, Upper Scorpius, Ophiuchi, and Orion
- A wide survey for circumstellar disks in the Lupus complex
- Low-mass pre--main-sequence stars in the Magellanic Clouds
- A Random Forest Approach to Identifying Young Stellar Object Candidates in the Lupus Star-Forming Region
- The disk of 2MASS 15491331-3539118 = GQ Lup C as seen by HST and WISE
- ALMA observations of the early stages of substellar formation in the Lupus 1 and 3 molecular clouds
- Velocity-Resolved [Ne III] from X-Ray Irradiated Sz 102 Microjets
- ISO-ChaI 52: a weakly-accreting young stellar object with a dipper light curve
- The Power of SOFIA/FORCAST in Estimating Internal Luminosities of Low Mass Class 0/I Protostars
- New members of the Lupus I cloud based on Gaia astrometry Physical and accretion properties from X-Shooter spectra